Fluctuating Dimension in a Discrete Model for Quantum Gravity Based on the Spectral Principle
Luiz C. de Albuquerque, Jorge L. deLyra, and Paulo Teotonio-Sobrinho

TL;DR
This paper introduces a discrete quantum gravity model based on the spectral principle, allowing topology, metric, and dimension to fluctuate, revealing two phases and a dynamical space-time dimension with an upper bound.
Contribution
It presents a novel discrete quantum gravity model where geometry and dimension are dynamical, and analyzes phase transitions and dimension bounds within this framework.
Findings
The model exhibits two phases with finite and divergent average number of points.
The critical point and exponent for the phase transition are computed.
An upper bound of <δ> < 2 for the expected space-time dimension is established.
Abstract
The spectral principle of Connes and Chamseddine is used as a starting point to define a discrete model for Euclidean quantum gravity. Instead of summing over ordinary geometries, we consider the sum over generalized geometries where topology, metric and dimension can fluctuate. The model describes the geometry of spaces with a countable number of points, and is related to the Gaussian unitary ensemble of Hermitian matrices. We show that this simple model has two phases. The expectation value , the average number of points in the universe, is finite in one phase and diverges in the other. We compute the critical point as well as the critical exponent of . Moreover, the space-time dimension is a dynamical observable in our model, and plays the role of an order parameter. The computation of is discussed and an upper bound is found, .
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